Fig. 3.
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Amplitudes, averaged for 4 < ℓ < 32, of the 𝒟ℓEE (diamond) and BB (square) power spectra versus frequency. Each plot presents the spectra of the Commander dust model (gray), our synchrotron estimate at 100 and 143 GHz (black), the CMB (orange), and the SRoll2 noise plus systematics (light brown). The three plots from left to right correspond to fsky = 80, 90, and 97%.
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